Neutron capture

Neutron capture at small neutron flux

At small mass number increases by one. In terms of a formula, this is written ¹⁹⁷Au(n,γ)¹⁹⁸Au. If thermal neutrons are used, this is called thermal capture.

The isotope ¹⁹⁸Au is a protons in the nucleus) rises by one.

The s-process mentioned above happens in the same way, but inside of stars.

Neutron capture at high neutron flux

The r-process happens inside stars if the neutron flux density is so high that the atomic nucleus has no time to decay via beta emission in between neutron captures. The mass number therefore rises by a large amount while the atomic number (i.e., the element) stays the same. Only afterwards, the highly unstable nuclei decay via many β^- decays to stable or unstable nuclei of high atomic number.

Capture cross section

The absorption chemical element is the effective cross sectional area that an atom of that isotope presents to absorption, and is a measure of the probability of neutron capture. It is usually measured in "barns" (b).

Absorption cross section is often highly dependent on neutron moderation slows the neutron down from an original high energy.

The thermal energy of the nucleus also has an effect; as temperatures rise, Doppler broadening increases the chance of catching a resonance peak. In particular, the increase in U-238's ability to absorb neutrons with increasing temperature is a negative feedback mechanism that helps keep nuclear reactors under control.

Uses

Neutron capture can be used to remotely detect the chemical composition of materials. This is because different elements release different characteristic radiation when they absorb neutrons. This makes it useful in many fields related to mineral exploration and security.

See also

• Beta decay
• Gamma ray
• List of particles
• Neutron
• Neutron emission
• Neutron radiation
• Radioactivity
• Rays: γ — δ — ε
• p-process (proton capture)

http://ie.lbl.gov/ng.html Thermal Neutron Capture Data